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The Physical Basis of The Direction of Time (The Frontiers ...

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∑<br />

j<br />

¯F µν<br />

j<br />

:= ∑ j<br />

2.4 <strong>The</strong> Absorber <strong>The</strong>ory <strong>of</strong> Radiation 37<br />

1<br />

[<br />

]<br />

F µν<br />

ret,j<br />

2<br />

+ F µν<br />

adv,j<br />

−→ 0 , (2.38)<br />

constitutes their cosmic absorber condition. Since the retarded or advanced<br />

fields vanish by definition in the asymptotic past or future, respectively, so<br />

must their time-reversed partner because <strong>of</strong> (2.38), and hence also their asymmetric<br />

combination. Wheeler and Feynman then concluded by means <strong>of</strong> the<br />

homogeneous Maxwell equations that the total asymmetric field would vanish<br />

everywhere. This is just the required ‘boundary’ condition.<br />

However, the consistency <strong>of</strong> this procedure is very questionable. A similar<br />

problem would arise for an expanding and recollapsing Universe that<br />

were sandwiched between two thermodynamically opposite radiation eras (absorbers<br />

with opposite thermodynamical arrows <strong>of</strong> time) – see Sect. 5.3. As<br />

explained in Sect. 2.1, the compatibility <strong>of</strong> double-ended (two-time) boundary<br />

conditions is highly nontrivial – similar to an eigenvalue problem. This consistency<br />

problem is particularly severe for a universe that remains optically<br />

transparent and thus preserves information contained in the radiation such as<br />

light (Davies and Twamley 1993).<br />

In contrast to the physical absorbers <strong>of</strong> Sect. 2.2, the new absorber condition<br />

is symmetric under time reversal. This fact led to many misunderstandings.<br />

For example, rather than adding the vanishing antisymmetric term to<br />

(2.36), one might as well subtract it in order to obtain the time-reversed representation<br />

ma µ i = e ∑<br />

i F µν<br />

adv,j (zσ i )v i,ν − e [<br />

]<br />

i<br />

F µν<br />

ret,i<br />

2<br />

(zσ i ) − F µν<br />

adv,i (zσ i ) v i,ν . (2.39)<br />

j(≠i)<br />

Although it is as correct as (2.37) under the absorber condition, (2.39) describes<br />

advanced actions and a radiation reaction that leads to reverse damping<br />

(exponential acceleration).<br />

<strong>The</strong>refore, Wheeler and Feynman’s absorber condition cannot explain the<br />

observed radiation arrow. Neither (2.37) nor (2.39) would describe the local<br />

empirical situation, which requires in general that only a limited number <strong>of</strong><br />

‘obvious sources’ contribute noticeably to the retarded sum (2.37). Otherwise,<br />

retardation would never have been recognized. This means that the retarded<br />

contribution <strong>of</strong> all ‘other’ sources (those which form the true universal absorber)<br />

must interfere destructively (see Fig. 2.7):<br />

∑<br />

F µν<br />

ret,i ≈ 0 ‘inside’ universal absorber . (2.40)<br />

i ∈ absorbers<br />

This is possible (except for the remaining thermal radiation) if the absorber<br />

particles approach thermal equilibrium by means <strong>of</strong> collisions after having<br />

been accelerated by retarded fields. <strong>The</strong>refore, one cannot expect<br />

∑<br />

F µν<br />

adv,i<br />

≈ 0 ‘inside’ universal absorber (2.41)<br />

i ∈ absorbers

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